Simulation of sigmoid structure and filament eruption of AR11283 using a three-dimensional data-driven magnetohydrodynamic model

S. T. Wu; Chaowei Jiang; Xueshang Feng; Qiang Hu; Yang Liu

doi:10.1017/S1743921313011587

Simulation of sigmoid structure and filament eruption of AR11283 using a three-dimensional data-driven magnetohydrodynamic model

S. T. Wu
, Chaowei Jiang
, Xueshang Feng
, Qiang Hu
, Yang Liu

University of Alabama in Huntsville
CAS - National Space Science Center
Stanford University

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

Abstract

This paper describes an MHD simulation of an observed Sigmoid in AR 11283 from its formation to eruption. The Non-linear Force Free MHD model (Jiang and Feng, 2012) and the data-driven active region evolution model (Wu et al., 2006; Jiang et al. 2013) together with the SDO/HMI magnetograms are used. We show the successful simulation results of the eruption of a flux-rope structure.

Original language	English
Title of host publication	Nature of Prominences and their Role in Space Weather
Publisher	Cambridge University Press
Pages	466-467
Number of pages	2
Edition	S300
ISBN (Print)	9781107045194
DOIs	https://doi.org/10.1017/S1743921313011587
State	Published - Jun 2013
Externally published	Yes

Publication series

Name	Proceedings of the International Astronomical Union
Number	S300
Volume	8
ISSN (Print)	1743-9213
ISSN (Electronic)	1743-9221

Keywords

Active region
MHD simulation
Magnetogram
Sigmoid

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10.1017/S1743921313011587

Cite this

Wu, S. T., Jiang, C., Feng, X., Hu, Q., & Liu, Y. (2013). Simulation of sigmoid structure and filament eruption of AR11283 using a three-dimensional data-driven magnetohydrodynamic model. In Nature of Prominences and their Role in Space Weather (S300 ed., pp. 466-467). (Proceedings of the International Astronomical Union; Vol. 8, No. S300). Cambridge University Press. https://doi.org/10.1017/S1743921313011587

@inproceedings{5090987ed51e4b76ab607f782d532471,

title = "Simulation of sigmoid structure and filament eruption of AR11283 using a three-dimensional data-driven magnetohydrodynamic model",

abstract = "This paper describes an MHD simulation of an observed Sigmoid in AR 11283 from its formation to eruption. The Non-linear Force Free MHD model (Jiang and Feng, 2012) and the data-driven active region evolution model (Wu et al., 2006; Jiang et al. 2013) together with the SDO/HMI magnetograms are used. We show the successful simulation results of the eruption of a flux-rope structure.",

keywords = "Active region, MHD simulation, Magnetogram, Sigmoid",

author = "Wu, \{S. T.\} and Chaowei Jiang and Xueshang Feng and Qiang Hu and Yang Liu",

year = "2013",

month = jun,

doi = "10.1017/S1743921313011587",

language = "英语",

isbn = "9781107045194",

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publisher = "Cambridge University Press",

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pages = "466--467",

booktitle = "Nature of Prominences and their Role in Space Weather",

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}

Wu, ST, Jiang, C , Feng, X, Hu, Q & Liu, Y 2013, Simulation of sigmoid structure and filament eruption of AR11283 using a three-dimensional data-driven magnetohydrodynamic model. in Nature of Prominences and their Role in Space Weather. S300 edn, Proceedings of the International Astronomical Union, no. S300, vol. 8, Cambridge University Press, pp. 466-467. https://doi.org/10.1017/S1743921313011587

Simulation of sigmoid structure and filament eruption of AR11283 using a three-dimensional data-driven magnetohydrodynamic model. / Wu, S. T.; Jiang, Chaowei ; Feng, Xueshang et al.
Nature of Prominences and their Role in Space Weather. S300. ed. Cambridge University Press, 2013. p. 466-467 (Proceedings of the International Astronomical Union; Vol. 8, No. S300).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

TY - GEN

T1 - Simulation of sigmoid structure and filament eruption of AR11283 using a three-dimensional data-driven magnetohydrodynamic model

AU - Wu, S. T.

AU - Jiang, Chaowei

AU - Feng, Xueshang

AU - Hu, Qiang

AU - Liu, Yang

PY - 2013/6

Y1 - 2013/6

N2 - This paper describes an MHD simulation of an observed Sigmoid in AR 11283 from its formation to eruption. The Non-linear Force Free MHD model (Jiang and Feng, 2012) and the data-driven active region evolution model (Wu et al., 2006; Jiang et al. 2013) together with the SDO/HMI magnetograms are used. We show the successful simulation results of the eruption of a flux-rope structure.

AB - This paper describes an MHD simulation of an observed Sigmoid in AR 11283 from its formation to eruption. The Non-linear Force Free MHD model (Jiang and Feng, 2012) and the data-driven active region evolution model (Wu et al., 2006; Jiang et al. 2013) together with the SDO/HMI magnetograms are used. We show the successful simulation results of the eruption of a flux-rope structure.

KW - Active region

KW - MHD simulation

KW - Magnetogram

KW - Sigmoid

UR - https://www.scopus.com/pages/publications/84891880973

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DO - 10.1017/S1743921313011587

M3 - 会议稿件

AN - SCOPUS:84891880973

SN - 9781107045194

T3 - Proceedings of the International Astronomical Union

SP - 466

EP - 467

BT - Nature of Prominences and their Role in Space Weather

PB - Cambridge University Press

ER -

Wu ST, Jiang C , Feng X, Hu Q, Liu Y. Simulation of sigmoid structure and filament eruption of AR11283 using a three-dimensional data-driven magnetohydrodynamic model. In Nature of Prominences and their Role in Space Weather. S300 ed. Cambridge University Press. 2013. p. 466-467. (Proceedings of the International Astronomical Union; S300). doi: 10.1017/S1743921313011587

Simulation of sigmoid structure and filament eruption of AR11283 using a three-dimensional data-driven magnetohydrodynamic model

Abstract

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